SCIENCE 8 TOPIC 5. The Six Factors that Set Planets Apart from the Stars.

Slides:



Advertisements
Similar presentations
Chapter 27.2 Models of the solar system
Advertisements

Topic IV: Motions of the Earth, Moon and Sun
Kepler’s laws.
Early Astronomers & Planetary Motion
Motions of the Earth, Moon and Sun
Goals Explain how accurate observations led to Heliocentric model Review contributions of Galileo and Kepler Explain Kepler’s Laws Explain Newton’s laws.
Topic: Models of the Universe Key Terms: Geocentric Theory Heliocentric Theory.
Early Models of the Universe. Pythagoreans (500 B.C.) Believed the stars, planets, sun, and moon were attached to crystalline spheres which rotated around.
Models of the Solar System. The observations that you have been making of the Sun, Moon and stars were the same observations made by early scientists.
Motions of the Earth and Sky Part II. Depending on the relative sizes and distances of the Sun and a moon, you might see an eclipse like this: Sun planet.
MOTIONS OF EARTH, MOON AND SUN
UNIT 4 SPACE EXPLORATION. Chapter 10 – The Universe Text page 350 ASTRONOMY – branch of physics which studies celestial bodies and the universe Any natural.
Introduction to Astronomy. How big, and small, is our universe, and how do scientists measure these vast differences? Scientific Notation—a convenient.
Bell Ringer 9/8 OPINION QUESTION – How do you believe the solar system was formed?
Web 1 Ancient Theories of Solar System 1.heliocentric theory 2. geocentric theory 3. Aristotle 4. Aristarchus 5. Ptolemy 6. Copernicus 7. Johannes Kepler.
Motions of Earth, Moon, and Sun. Apparent Motions of Celestial Objects An apparent motion is a motion that an object appears to make. Apparent motions.
Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 2.
Scientific Models & Kepler’s Laws Scientific Models We know that science is done using the Scientific Method, which includes the following steps : Recognize.
Origin of Modern Astronomy
Opening for today… Kepler’s Laws of Planetary Motion Objective: Students will explain planetary motion using gravitational laws.
Solar System Models Geocentric Model Earth Centered Moon, Sun, Planets, and Stars revolve around the Earth Feels right No observed parallax of stars.
History of Astronomy. Our Universe Earth is one of nine planets that orbit the sun The sun is one star in 100 billion stars that make up our galaxy- The.
Goals Explain how accurate observations led to Heliocentric model Explain retrograde motion Describe contributions of Copernicus, Tycho, Galileo, and.
Planetary Orbits The ancient Greeks (Aristotle and Plato) thought the only perfect shapes were the circle and line. All things fall in a line toward Earth,
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Kepler’s Laws of Planetary Motion. Debate on Planet Motions Geocentric or Heliocentric Universe.
Topic: Models of the Universe Key Terms: Geocentric Theory Heliocentric Theory.
Ch. 22 Origin of Modern Astronomy Sec. 1 Early Astronomy 200.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
Earth Science 22.1 Origins of Astronomy Origins of Astronomy.
Chapter 1: The Copernican Revolution. The Motions of the Planets The Birth of Modern Astronomy The Laws of Planetary Motion Newton’s Laws Summary of Chapter.
The Early History of Astronomy The ancient people saw seven celestial bodies moving through the stars; Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn.
Model of the Solar System. Who is This Greek Guy?
ASTRONOMY AND THE BIRTH OF MODERN SCIENCE. ANCIENT ASTRONOMY Human Survival  Predict when to plant crops Indian ruins line up with Summer and winter.
Ch 22 Astronomy. Ancient Greeks 22.1 Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation.
Astronomy Questions
CHAPTER 22 THE SUN and ITS SOLAR SYSTEM II. Observing the Solar System.
 Everything in outer space  Stars  Planets  Comets  Asteroids & Meteors  Solar System vs Galaxy vs Universe  What’s the difference?  SIZE?!
TOPIC #1: Chapter 22 Origin of Modern Astronomy. Section 1: Early Astronomy Astronomy is the science that studies the universe. The “Golden Age” of early.
Astronomy Final Review. Geocentric Model --Earth is in the center of the system and everything revolves around it.
Ch. 29 The Solar System.
 Definition - Earth is at the center of the solar system being orbited by the Sun and other planets  (sketch a picture of a geocentric solar system)
Geocentric Model Heliocentric Model Did you know???? (do not write)  It wasn’t until 1851 that experimental proof of the motion of Earth was found.
The planets 12/1/14.
Don’t Write What is in Green. Geocentric Model.
Introduction to Classical Astronomy Mr. Ross Brown Brooklyn School for Law and Technology.
Models of the Solar System Ch 27.2 Page 691 Early models  Around 2,000 years ago, Aristotle suggested the earth- centered or geocentric model of the.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
CHAPTER 27 SECTION 2 EARTH AND SPACE AUSTIN HIGH SCHOOL Models of the Solar System.
Outer Space Chapters 25 and Solar System Made up of: Sun (a.k.a. star) Planets Moons (yes plural) Other small objects.
Ancient Greeks Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies.
Think About It: For 1,700 years what did we believe about the Earth and the Sun and their motions? Why did we believe that? For 1,700 years what did we.
Our View of the Universe
How does the geocentric model differ from the heliocentric model?
Bellwork Who is credited with the revolutionary model of a HELIOCENTRIC solar system? A. Aristotle B. Ptolemy C. Galileo D. Copernicus The planets loop.
Earths Motions Objectives:
Geocentric/Heliocentric
TOPIC 3 EARTH MOTIONS.
MODELS OF THE SOLAR SYSTEM
Part 1: Planets and SS models Part 2: Kepler’s Laws of Motion
Model of the Solar System
Part 1: Planets and SS models Part 2: Kepler’s Laws of Motion
22.1 Early Astronomy.
Geocentric vs. Heliocentric Models
What is the universe Part 2 Motion in Space
Chapter 3 Analyzing Scales and Motions of the Universe
The Laws of Planetary Motion
Lesson 2 Models of the Universe
Astronomy Terms-Copy & define these terms to be placed in flipbook
Kepler’s Laws of Planetary Motion
Presentation transcript:

SCIENCE 8 TOPIC 5

The Six Factors that Set Planets Apart from the Stars

1. Planets have the same westward drift as the stars, but slightly slower than the stars. Venus

2. Planets appear to show retrograde motion (movement in a backward direction).

3. A planet’s distance from the earth changes over time. 4. A planet’s diameter changes over time.

5. A planet’s brightness changes over time.

6. Planets have surface features that change over time.

The Geocentric Model

Why the Geocentric Model was a “bad dog”: 1.Future positions of planets weren’t predictable 2.Terrestrial motions were not accounted for 3.The model became too complicated

The Heliocentric Model Solved all the problems...except for...

“Little problems not explained by the Heliocentric Model: 1.The apparent differences in the sun’s diameter 2.The varying speed of the earth in it’s orbit 3.The moon’s speed and diameter changes

Retrograde Motion of the Planets

How the Coriolis Effect Supported the Heliocentric Model (projectiles)

How the Coriolis Effect Supported the Heliocentric Model (ocean currents)

How the Pendulum’s Movement Supported the Heliocentric Model

How the Pendulum’s Movement Supported the Heliocentric Model Rotating on an axis helped explain the change in terrestrial features

The Ellipse: an orbit that appears as a flattened circle

How Did the Ellipse Solved the Earlier Problems with the Heliocentric model?

The ellipse solved the problems with the apparent differences in the sun’s diameter, the varying speed of the earth, and with the moon’s apparent speed and diameter changes.

The Law of Equal Areas states that equal areas of space are swept by a planet during equal amounts of time.

Why the Moon (or any satellite) Stays in Orbit Around the Earth